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Дата изменения: Wed Feb 3 21:01:00 2016
Дата индексирования: Sun Apr 10 02:13:36 2016
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The Sunspot Observer - The solar regions - The description of the solar regions

Statistics of sunspot activity

NOAA 10100 - NOAA 10199
The description of the solar regions

NOAA 10100The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 1.09 to 12.09.02 along the high latitudes of the Southern hemisphere. In the first days the total region's area reached 200 m.s.h. Neighbouring the central meridian the sunspot had bifurcated and began decay.
 
NOAA 10101The fine sunspots crossed the Sun disc since 1.09 to 11.09.02 along the equator.
 
NOAA 10102The fine sunspot with symmetrical penumbra was observed at the low latitudes of the Northern hemisphere since 1.09 to 5.09.02, in the Eastern part of the Sun disc.
 
NOAA 10103The spreading bipolar group crossed the Sun disc since 3.09 to 15.09.02 along the mid latitudes of the Northern hemisphere. In the evolution's peak the total area of the region exceeded 500 m.s.h., and it was counted 40-45 sunspots in the group.
 
NOAA 10104The insignificant sunspots were observed at the tenth parallel of the Northern hemisphere since 7.09 to 13.09.02.
 
NOAA 10105The giant sunspot with asymmetrical penumbra was crossed the Sun disc since 7.09 to 20.09.02 along the low latitudes of the Southern hemisphere. Many fine spots and pores were observed neighbouring the sunspot. The region was classified as a closed multipole. On 10.09 the total group's area had exceeded 1500 m.s.h. It was counted more 50 sunspots in the group.
 
NOAA 10106The short-time sunspots were marked at the 27th parallel of the Northern hemisphere on 8.09 and 9.09.02, in the Eastern part of the Sun disc.
 
NOAA 10107The perceptible bipolar group crossed the Sun disc since 8.09 to 20.09.02 along the tenth parallel of the Northern hemisphere. The head and tail parts of the group consisted of small sunspots with penumbraes. Several pores connected two parts of the group. Neighbouring the central meridian the total region's area reached 200 m.s.h., and it was counted 20-25 sunspots and pores in the group. After intersection of the central meridian the tail sunspots began decay, and one of the head sunspots assumed symmetrical form and reached the Western limb.
 
NOAA 10108The fine sunspots were noticed at the 24th parallel of the Southern hemisphere since 9.09 to 12.09.02, in the Eastern part of the Sun disc.
 
NOAA 10109The small bipolar group was marked to the West from the large region 10105 since 10.09 to 14.09.02.
 
NOAA 10110The fine bipolar sunspots were observed at the high latidudes of the Northern hemisphere since 10.09 to 18.09.02. The bipole had almost meridianal direct.
 
NOAA 10111The bipolar pores were noticed at the tenth parallel of the Northern hemisphere since 12.09 to 14.09.02.
 
NOAA 10112The short-time pore was marked in the Sun disc's center on 12.09 and 13.09.02.
 
NOAA 10113The high latitude one-day pore was noticed in the Northern hemisphere on 12.09.02, in the Western part of the Sun disc.
 
NOAA 10114The tail part of the large region 10105 was classified as a separate bipole since 14.09 to 21.09.02. The new group consisted of perceptible sunspot with symmetrical penumbra, and many fine sunspots were settled behind it and were embedded into several pieces of penumbra. In the first days the total region's area exceeded 300 m.s.h., and it was counted more 30 sunspots in the group.
 
NOAA 10115The perceptible bipolar group crossed the Sun disc since 13.09 to 23.09.02 along the equator. The head and tail sunspots had developed penumbraes. Neighbouring the central meridian the group lined into an unstable chain of developed sunspots which began soon crumble. The maximal total area of the region reached 250 m.s.h., and it was counted more 20 sunspots in the group. In several days the tail part of the group decayed, and the head sunspot assumed symmetrical form and reached the Western limb on 23.09.
 
NOAA 10116The insignificant bipolar sunspots were marked at the mid latitudes of the Northern hemisphere since 15.09 to 21.09.02.
 
NOAA 10117The big sunspot with symmetrical penumbra crossed the Sun disc since 15.09 to 27.09.02 along the tenth parallel of the Southern hemisphere.
 
NOAA 10118The short-time pores were marked on 16.09 and 17.09.02 in the central part of the Sun disc.
 
NOAA 10119The new bipolar group had appeared at the mid latitudes of the Southern hemisphere on 15.09.02, in the Eastern part of the Sun disc. The impetuous evolution's process started in the head sunspot with symmetrical penumbra, and new sunspots with powerful penumbraes appeared behind it. In several days the total region's area increased in tens times and exceeded 600 m.s.h. It was counted 30-40 sunspots in the group. On 25.09 the new multipole had come to the Western limb.
 
NOAA 10120The fine bipolar sunspots were marked to the South from the big sunspot 10117 since 16.09 to 21.09.02.
 
NOAA 10121The fine sunspot with symmetrical penumbra was observed to the South-East from the big sunspot 10117 since 16.09 to 25.09.02.
 
NOAA 10122The fine sunspot with symmetrical penumbra crossed the Sun disc since 17.09 to 28.09.02 along the mid latitudes of the Southern hemisphere.
 
NOAA 10123The fine bipolar sunspots were observed since 17.09 to 25.09.02 to the East from the big region 10119.
 
NOAA 10124The short-time near equatorial sunspots were marked on 18.09 and 19.09.02 in the Western part of the Sun disc.
 
NOAA 10125The fine sunspots crossed the Sun disc since 18.09 to 30.09.02 along the low latitudes of the Southern hemisphere.
 
NOAA 10126The fine bipolar group was observed at the high latitudes of the Southern hemisphere since 19.09 to 24.09.02.
 
NOAA 10127The perceptible bipolar group was observed at the mid latitudes of the Southern hemisphere since 20.09 to 27.09.02. The head and tail parts of the group consisted of several nearby sunspots with penumbraes. The sunspots regular changed form and combination. The total region's area reached 200 m.s.h.
 
NOAA 10128The short-time sunspots were marked at the tenth parallel of the Northern hemisphere on 20.09 and 21.09.02, in the Eastern part of the Sun disc.
 
NOAA 10129The insignificant bipolar sunspots crossed the Sun disc since 22.09 to 30.09.02 along the 27th parallel of the Sun disc.
 
NOAA 10130The new bipolar group had appeared at the low latitudes of the Northern hemisphere on 21.09.02, in the Eastern part of the Sun disc. The bipole was slowly extending. Neighbouring the central meridian the total area reached 250 m.s.h. The head sunspot had big asymmetrical penumbra, and fine tail sunspots were enclosed into general oblong penumbra. Then the tail sunspots began decay, and the head sunspot assumed symmetrical form and had come to the Western limb on 2.10.
 
NOAA 10131The insignificant sunspots were observed at the low latitudes of the Southern hemisphere since 22.09 to 27.09.02.
 
NOAA 10132The new compact bipole had appeared at the high latitudes of the Northern hemisphere on 22.09.02, neighbouring the central meridian. The group consisted of several perceptible sunspots which were enclosed into general irregular penumbra. In the evolution's peak the total region's area reached 400 m.s.h. On 29.09 the new group reached the Western limb.
 
NOAA 10133The insignificant bipolar formation was observed at the 25th parallel of the Southern hemisphere since 22.09 to 27.09.02.
 
NOAA 10134The spreading bipolar group crossed the Sun disc since 24.09 to 6.09.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of developed sunspots and pores. Neighbouring the central meridian the total region's area exceeded 300 m.s.h., and it was counted more 30 sunspots in the group.
 
NOAA 10135The insignificant bipolar sunspots were observed at the 25th parallel of the Southern hemisphere since 27.09 to 30.09.02.
 
NOAA 10136The fine sunspots were marked at the high latitudes of the Southern hemisphere since 29.09 to 1.10.02, in the Western part of the Sun disc.
 
NOAA 10137The developed bipolar group crossed the Sun disc since 28.09 to 10.10.02 along the high latitudes of the Southern hemisphere. In the first days the new bipole was quickly extended. Neighbouring the central meridian the total region's area exceeded 300 m.s.h., and it was counted 25-30 sunspots in the group. Then the tail part of the group began decay, and the head sunspot assumed symmetrical form and reached the Western limb.
 
NOAA 10138The fine sunspots were marked neighbouring the bipolar region 10134 since 24.09 to 5.10.02.
 
NOAA 10139The big multipole crossed the Sun disc since 2.10 to 15.10.02 along the tenth parallel of the Northern hemisphere. Two sunspots with general penumbra were as a base of the group. The oblong sunspot had large sizes, and the asymmetrical sunspot had perceptible sizes. Two sunspots were like exclamation point. Many small sunspots and pores were observed neighbouring the sunspots. The maximal total area of the region exceeded 600 m.s.h., and it was counted more 40 sunspots in the group.
 
NOAA 10140The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 4.10 to 17.10.02 along the low latitudes of the Southern hemisphere. The rest of the bipolar region 10114. From time to time the total sunspot's area reached 200 m.s.h.
 
NOAA 10141The fine bipolar sunspots were marked at the mid latitudes of the Southern hemisphere since 5.10 to 9.10.02.
 
NOAA 10142The fine sunspot with symmetrical penumbra crossed the Sun disc since 5.10 to 11.10.02 along the low latitudes of the Northern hemisphere.
 
NOAA 10143The fine bipolar group was marked at the mid latitudes of the Southern hemisphere since 7.10 to 10.10.02, in the Western part of the Sun disc.
 
NOAA 10144The new bipolar group had appeared at the mid latitudes of the Northern hemisphere on 7.10.02, in the Eastern part of the Sun disc. The head sunspot's penumbra had formed in the first day, and the tail sunspot's penumbra appeared in next day. Then the tail part of the group began crush and gradually decay. The maximal total area of the region exceeded 100 m.s.h., then it was counted more twenty sunspots in the group. On 17.10 the group had come to the Western limb.
 
NOAA 10145The small sunspot with symmetrical penumbra crossed the Sun disc since 8.10 to 20.10.02 along the mid latitudes of the Northern hemisphere. From time to time pores with opposite magnetic polarity appeared neighbouring the sunspot.
 
NOAA 10146The fine group was observed at the Eastern district of the bipolar region 10140 since 8.10 to 12.10.02.
 
NOAA 10147The near equatorial bipolar pores were marked on 9.10 and 10.10.02 in the Eastern part of the Sun disc.
 
NOAA 10148The fine sunspot with symmetrical penumbra crossed the Sun disc since 9.10 to 19.10.02 along the high latitudes of the Southern hemisphere.
 
NOAA 10149The big multipole crossed the Sun disc since 8.10 to 21.10.02 along the mid latitudes of the Northern hemisphere. The sunspot with big asymmetrical penumbra was as a base of the group. In the first days a chain of small sunspots appeared to the South from the sunspot which began extend and develop. More developing sunspot stood out in the head part of the chain which was situated to the South-West from the base sunspot of the group. In time the tail part of the chain decayed, and all the group assumed bipolar configuration of two developed and nearby sunspots. The total region's area exceeded 300 m.s.h. From time to time it was counted more 40 sunspots in the group.
 
NOAA 10150The short-time sunspots were marked in the central part of the Sun disc since 8.10 to 10.10.02.
 
NOAA 10151The recurrent pore was observed on 8.10, 9.19, 17.10 and 18.10.02 at the mid latitudes of the Southern hemisphere.
 
NOAA 10152The short-time bipolar sunspots were noticed on 10.10 and 11.10.02 to the North-East from the big region 10139.
 
NOAA 10153The short-time near equatorial pore was marked on 10.10.02 in the Eastern part of the Sun disc.
 
NOAA 10154The fine bipolar sunspots crossed the Sun disc since 10.10 to 20.10.02 along the mid latitudes of the Southern hemisphere.
 
NOAA 10155The fine bipolar sunspots were noticed on 11.10 and 12.10.02. not far the Western limb.
 
NOAA 10156The short-time sunspots were marked at the low latitudes of the Northern hemisphere since 10.10 to 13.10.02, in the Eastern part of the Sun disc.
 
NOAA 10157The short-time sunspots were marked at the mid latitudes of the Northern hemisphere since 11.10 to 14.10.02, in the Eastern part of the Sun disc.
 
NOAA 10158The recurrent group crossed the Sun disc since 12.10 to 24.10.02 along the low latitudes of the Southern hemisphere. In the first days the group was as a perceptible sunspot with symmetrical penumbra. Then many fine sunspots with opposite magnetic polarity appeared to the North from the sunspot, and its had fast development. From time to time the total region's area reached 150 m.s.h., and it was counted 20-25 sunspots in the group.
 
NOAA 10159The sunspot with asymmetrical penumbra was spliting up into three fine and lined spots. The region crossed the Sun disc since 13.10 to 22.10.02 along the mid latitudes of the Southern hemisphere.
 
NOAA 10160The perceptible bipolar group crossed the Sun disc since 13.10 to 24.10.02 along the high latitudes of the Southern hemisphere. The bipole was quickly developing and decaying. The maximal total area of the region exceeded 200 m.s.h., and it was counted 25-30 sunspots in the group.
 
NOAA 10161The short-time sunspots were marked at the low latitudes of the Northern hemisphere since 15.10 to 18.10.02.
 
NOAA 10162The large bipolar group crossed the Sun disc since 17.10 to 31.10.02 along the 25th parallel of the Northern hemisphere. The bipole consisted of the imposing head sunspot with symmetrical penumbra and the big tail part which had complex structure. Neighbouring the central meridian the main tail sunspots built fanciful form like a three-leaf flower. In the evolution peak the total region's area exceeded 1000 m.s.h., and it was counted 50-60 sunspots in the group.
 
NOAA 10163The short-time bipolar pores were noticed at the high latitudes of the Southern hemisphere on 18.10.02, to the West from the central meridian.
 
NOAA 10164The insignificant recurrent sunspots were observed at the tenth parallel of the Northern hemisphere since 19.10 to 25.10.02, in the Eastern part of the Sun disc.
 
NOAA 10165The perceptible double sunspot with oblong penumbra crossed the Sun disc since 19.10 to 1.11.02, along the high latitudes of the Northern hemisphere. The maximal total area of the region exceeded 250 m.s.h. The sunspot was slowly diminished and assumed more symmetrical form.
 
NOAA 10166The short-time pore was noticed on 23.10.02 in the Sun disc's center.
 
NOAA 10167The small sunspot with symmetrical penumbra crossed the Sun disc since 23.10 to 3.11.02 along the mid latitudes of the Northern hemisphere.
 
NOAA 10168The sunspot with symmetrical penumbra was marked at the 25th of the Northern hemisphere on 24.10 and 25.10.02, near the Western limb.
 
NOAA 10169The small bipolar group crossed the Sun disc since 24.10 to 1.11.02 along the high latitudes of the Southern hemisphere. The bipole consisted of two fine, nearby sunspots with penumbraes. In the first days the total region's area reached 100 m.s.h.
 
NOAA 10170The fine bipolar sunspots were observed hardly to the North from the region 10169 since 25.10 to 30.10.02.
 
NOAA 10171The fine sunspot with penumbra crossed the Sun disc since 25.10 to 2.11.02 along the tenth parallel of the Northern hemisphere.
 
NOAA 10172The fine sunspot with symmetrical penumbra was observed at the mid latitudes of the Southern hemisphere since 26.10 to 30.10.02, in the Eastern part of the Sun disc.
 
NOAA 10173The fine bipolar group was marked at the mid latitudes of the Southern hemisphere since 28.10 to 30.10.02, near the Western limb.
 
NOAA 10174The small bipolar chain was observed at the 25th parallel of the Southern hemisphere since 28.10 to 3.11.02, in the Eastern part of the Sun disc. There was a sunspot with fine asymmetrical penumbra in the chain's middle.
 
NOAA 10175The opened bipolar group crossed the Sun disc since 28.10 to 8.11.02, along the mid latitudes of the Southern hemisphere. The head sunspot had perceptible symmetrical penumbra, the fine tail sunspot slowly decayed. Many fine spots and pores were observed around the sunspots. In the evolution's peak the total region's area exceeded 150 m.s.h., and it was counted more twenty sunspots in the group.
 
NOAA 10176The sunspot with symmetrical penumbra crossed the Sun disc since 29.10 to 11.11.02, along the tenth parallel of the Northern hemisphere. The rest of the big bipolar region 10139. The total sunspot's area exceeded 100 m.s.h.
 
NOAA 10177The perceptible bipolar group crossed the Sun disc since 30.10 to 11.11.02, along the mid latitudes of the Northern hemisphere. The bipole consisted of the big head sunspot with asymmetrical penumbra and many fine sunspots and pores behind it. On 5.11 the head sunspot began bifurcated, and then the newly formated sunspots slowly moved away along the meridianal direct. The total region's area reached 400 m.s.h., and it was counted 25-30 sunspots in the group.
 
NOAA 10178The new bipolar group was observed since 31.10 to 5.11.02 in the Western part of the Sun disc. The bipole consisted of perceptible sunspot with penumbra and string of fine spots and pores which lined behind it. From time to time the total region's area reached 100 m.s.h.
 
NOAA 10179The fine near equatorial sunspot with symmetrical penumbra was observed since 1.11 to 7.11.02.
 
NOAA 10180The big multipole crossed the Sun disc since 1.11 to 13.11.02 along the tenth parallel of the Southern hemisphere. The group consisted of many sunspots with different sizes which were scattered at a latitude on considerable distance. In the evolution's peak the total area of the region exceeded 500 m.s.h., and it was counted more 50 sunspots in the group.
 
NOAA 10181The short-time bipolar sunspots were noticed at the Western district of the big region 10180 since 2.11 to 5.11.02.
 
NOAA 10182The small group was observed to the South-East from the region 10180 since 2.11 to 14.11.02. The head sunspot had stable symmetrical penumbra. The fine tail sunspot quickly decayed.
 
NOAA 10183The short-time sunspots were marked on 3.11 and 4.11.02 to the West from the central meridian.
 
NOAA 10184The fine sunspot were noticed on 2.11 and 3.11.02 near the Eastern limb.
 
NOAA 10185The perceptible nuclears were united by general asymmetrical penumbra. The region crossed the Sun disc since 3.11 to 15.11.02, along the mid latitudes of the Southern hemisphere. In the first days the total group's area reached 300 m.s.h.
 
NOAA 10186The fine bipolar sunspots were observed to the East from the region 10177 since 5.11 to 8.11.02.
 
NOAA 10187The short-time sunspots were noticed in the central part of the Sun disc since 5.11 to 8.11.02.
 
NOAA 10188The briskly developing bipolar group was marked at the tenth parallel of the Northern hemisphere since 5.11 to 11.11.02. The maximal total area of the region reached 150 m.s.h., and it was counted twenty sunspots in the group.
 
NOAA 10189The fine sunspots crossed the Sun disc since 5.11 to 13.11.02 along the mid latitudes of the Northern hemisphere.
 
NOAA 10190The fine high latitude sunspots crossed the Sun disc in the Southern hemisphere since 7.11 to 15.11.02.
 
NOAA 10191The big multipolar group crossed the Sun disc since 8.11 to 21.11.02. along the high latitudes of the Southern hemisphere. The multipole consisted of many sunspots and pores which were enclosed by several big pieces of penumbra. The total region's area reached 600-700 m.s.h., and it was counted 60-70 sunspots in the group. Before set for the limb the group began decay.
 
NOAA 10192The new bipolar group had appeared on 11.11.02 neighbouring the central meridian. In the first days the sunspots were almost not noticeable. On 14.11 a small net had appeared in the place which was woven by fine sunspots and pores. In next day the structure turned into perceptible bipolar group which consisted of developed sunspots with penumbraes. The total region's area reached 500 m.s.h. On 19.11 the new group set for the limb.
 
NOAA 10193The fine recurrent sunspots were noticed at the Sun equator since 13.11 to 16.11.02.
 
NOAA 10194The fine bipolar group was marked behind the big region 10191 since 13.11 to 17.11.02.
 
NOAA 10195The perceptible bipolar group crossed the Sun disc since 13.11 to 26.11.02, along the mid latitudes of the Southern hemisphere. The head sunspot had stable penumbra with moderate sizes, the tail part consisted of two sunspots with penumbraes which were parted by a longitude and gradually decayed. The total region's area reached 300-350 m.s.h.
 
NOAA 10196The short-time sunspots were noticed at the high latitudes of the Southern hemisphere on 14.11 and 15.11.02, in the Western part of the Sun disc.
 
NOAA 10197The symmetrical penumbra with impressive penumbra crossed the Sun disc since 14.11 to 27.11.02, along the 25th parallel of the Northern hemisphere. The rest of the large region 10162. The total sunspot's area reached 300-400 m.s.h.
 
NOAA 10198The big bipolar group crossed the Sun disc since 15.11 to 29.11.02, along the mid latitudes of the Southern hemisphere. The head part of the group consisted of double sunspot with general penumbra and had imposing sizes. A long string of fine sunspots and pores lined behind the sunspot which was slowly decaying. From time to time the total region's area exceeded 600 m.s.h.
 
NOAA 10199The fine bipolar formation was marked to the East from the large sunspot 10197 since 18.11 to 26.11.02.
 












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